Table 1.
Basic radio properties of the ten new GRQs.
| Sr.No | RA | Dec | z | Size | Size | S1400 | P1400 | S150 | P150 |  |
QJet | Morphology |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (h min s) | (° ′ ″) | (′) | (Mpc) | (mJy) | (1025 W Hz−1) | (mJy) | (1025 W Hz−1) | (1043 erg s−1) | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) | (13) |
| 1 | 08 54 17.34 | 29 23 14.4 | 0.67075 ± 0.00007 | 1.81 | 0.78 | 121 ± 4 | 21.4 ± 1.2 | – | – | – | – | II |
| 2 | 09 31 10.90 | 54 49 38.0 | 1.18915 ± 0.00026 | 3.03 | 1.55 | 20 ± 1 | 13.4 ± 1.2 | – | – | – | – | II |
| 3 | 09 51 22.08 | 02 15 56.1 | 1.18890 ± 0.00037 | 1.70 | 0.87 | 11 ± 1 | 7.6 ± 0.9 | – | – | – | – | II |
| 4 | 10 51 52.62 | 02 24 02.7 | 1.36687 ± 0.00065 | 1.51 | 0.78 | 12 ± 1 | 11.9 ± 1.5 | 66 ± 15 | 63.3 ± 15.3 | 0.75 ± 0.25 | 21.1 ± 5.1 | II |
| 5 | 12 33 53.07 | 58 24 05.9 | 1.51526 ± 0.00031 | 1.51 | 0.79 | 46 ± 2 | 29.5 ± 2.9 | 53 ± 12 | 34.3 ± 8.2 | 0.07 ± 0.23 | 11.4 ± 2.7 | II |
| 6 | 12 36 04.51 | 10 34 49.2 | 0.66668 ± 0.00005 | 1.70 | 0.74 | 221 ± 7 | 35.6 ± 1.9 | 749 ± 151 | 121.3 ± 24.9 | 0.55 ± 0.21 | 40.2 ± 8.3 | II |
| 7 | 13 22 17.27 | 29 45 51.3 | 1.71883 ± 0.00066 | 1.61 | 0.84 | 75 ± 3 | 69.0 ± 7.0 | 113 ± 24 | 105.2 ± 24.4 | 0.19 ± 0.22 | 34.9 ± 8.1 | II |
| 8 | 15 21 13.37 | 44 08 33.8 | 1.06050 ± 0.00042 | 1.40 | 0.70 | 22 ± 1 | 11.2 ± 0.9 | – | – | – | – | II |
| 9 | 16 04 13.72 | 47 20 44.2 | 1.44235 ± 0.00052 | 1.37 | 0.71 | 20 ± 1 | 14.4 ± 1.7 | 39 ± 10 | 28.8 ± 7.9 | 0.31 ± 0.27 | 9.6 ± 2.7 | II |
| 10 | 16 22 01.90 | 44 10 09.7 | 1.29678 ± 0.00031 | 1.66 | 0.86 | 11 ± 1 | 8.9 ± 1.1 | – | – | – | – | II |
Notes. Columns (2) and (3) represent the right ascension (RA) in HMS (h min s) and declination (Dec) in DMS (° ′ ″) of the host of the GRQs. Column (4) lists the spectroscopic redshifts of the hosts. Columns (5) and (6) show the angular size and the projected linear sizes of the sources in arcminutes and megaparsecs, respectively. Columns (7) and (9) list the integrated flux densities (Sν), and Cols. (8) and (10) the total power Pν of the sources at 1400 MHz and 150 MHz, respectively. Column (11) states the 
, which is the two-point spectral index between 1400 MHz (NVSS) and 150 MHz (TGSS). Column (12) contains the jet kinetic power of the sources. Column (13) lists the morphological type of the sources (with ‘II’ representing FR-II type).
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